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- W2999543485 abstract "New H Fabry-Perot interferometer observations of the Virgo cluster spiral galaxy NGC 4522 are presented. A ve- locity field up to a radius of 60 00 was obtained. The observed rotation curve is symmetric. It is not perturbed in the inner disk. For radii > 50 00 it shows a solid body rotation. We compare these data with a numerical model which includes the effects of ram pressure stripping. The model can reproduce the main char- acteristics of the H emission distribution and velocity field. We therefore conclude that the stripping event which caused the Hi deficiency and the distorted H distribution and velocity field has been due to ram pressure. The closest passage of the galaxy to the cluster center is estimated to be 6.5 10 8 yr ago. The observed recent star formation is due to the re-accretion of gas clouds which were accelerated to velocities below the escape velocity during the stripping event. Furthermore, the gas which is located at radii > 60 00 is part of an asymmetric expanding ring" @default.
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- W2999543485 date "2000-12-18" @default.
- W2999543485 modified "2023-10-17" @default.
- W2999543485 title "The consequences of ram pressure stripping on the Virgo cluster spiral galaxy NGC 4522" @default.
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